Along similar lines, a canonical moment description of field theories has been
performed in [1]}, where the analog of (REF ) is the
Coleman–Weinberg potential [2]}. Here, we apply canonical
moment methods to a field theory motivated by spherically symmetric
gravitational systems, retaining independent quantum degrees of freedom such
as a field version of \(s\) . We therefore derive non-adiabatic or non-local
effects of quantum gravity.
